Phase Transitions, Shadows, and Microstructure of Kerr-anti-de Sitter Black Holes from Geometrothermodynamics

arXiv:2505.02389 · gr-qc, astro-ph.HE · Submitted 2025-05-05 · Read on arXiv

gr-qc, astro-ph.HE

Submitted: 2025-05-05

Updated: 2025-05-21

Terminology

• Phase Transitions — 31× in this paper · explained in 2 episodes
• Universality Class — 4× in this paper · explained in 2 episodes
• Consistency — 3× in this paper · explained in 3 episodes
• Conformal Field Theory — 1× in this paper
• Generalization — 1× in this paper · explained in 13 episodes
• Homogeneity — 1× in this paper · explained in 2 episodes

Sources

• Geometric Thermodynamics of Kerr-AdS black hole with a Cosmological Constant as State Variable
• Generalized Euler Equation from Effective Action: Implications for the Smarr Formula in AdS Black Holes
• Hyperscaling violating Schrodinger black holes in Einstein-Maxwell-scalar theory
• On Thermodynamic Stability of Black Holes. Part II: AdS Family of Solutions

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